[HTML][HTML] The 2024 release of the ExoMol database: molecular line lists for exoplanet and other hot atmospheres

J Tennyson, SN Yurchenko, J Zhang… - Journal of Quantitative …, 2024 - Elsevier
The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …

[HTML][HTML] Are These Planets or Brown Dwarfs? Broadly Solar Compositions from High-resolution Atmospheric Retrievals of∼ 10–30 M Jup Companions

JW Xuan, CC Hsu, L Finnerty, J Wang… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract Using Keck Planet Imager and Characterizer high-resolution (R∼ 35,000)
spectroscopy from 2.29 to 2.49 μm, we present uniform atmospheric retrievals for eight …

Fresh view of the hot brown dwarf HD 984 B through high-resolution spectroscopy

JC Costes, JW Xuan, A Vigan, J Wang… - Astronomy & …, 2024 - aanda.org
Context. High-resolution spectroscopy has the potential to drive a better understanding of
the atmospheric composition, physics, and dynamics of young exoplanets and brown …

The ESO SupJup Survey-II. The 12C/13C isotope ratios of three young brown dwarfs with CRIRES+

DG Picos, IAG Snellen, S de Regt, R Landman… - Astronomy & …, 2024 - aanda.org
Context. Young brown dwarfs exhibit atmospheric characteristics similar to those of super-
Jupiters, providing a unique opportunity to study planetary atmospheres. Atmospheric …

[HTML][HTML] Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy

CC Hsu, JJ Wang, JW Xuan, JB Ruffio… - The Astrophysical …, 2024 - iopscience.iop.org
We present the projected rotational velocity and molecular abundances for HD 33632 Ab
obtained via Keck Planet Imager and Characterizer (KPIC) high-resolution spectroscopy. HD …

Peering above the clouds of the warm Neptune GJ 436 b with CRIRES+

N Grasser, IAG Snellen, R Landman, DG Picos… - Astronomy & …, 2024 - aanda.org
Context. Exoplanets with masses between Earth and Neptune are amongst the most
commonly observed, yet their properties are poorly constrained. Their transmission spectra …

The ESO SupJup Survey. III. Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+

Y Zhang, DG Picos, S de Regt… - The Astronomical …, 2024 - iopscience.iop.org
High-resolution spectroscopic characterization of young super-Jovian planets enables
precise constraints on elemental and isotopic abundances of their atmospheres. As part of …

Atmospheric Characterization of the Super-Jupiter HIP 99770 b with KPIC

Y Zhang, JW Xuan, D Mawet, JJ Wang… - The Astronomical …, 2024 - iopscience.iop.org
Young, self-luminous super-Jovian companions discovered by direct imaging provide a
challenging test for planet formation and evolution theories. By spectroscopically …

Four HD 209458 b transits through CRIRES+: Detection of H2O and non-detections of C2H2, CH4, and HCN

D Blain, R Landman, P Mollière, J Dittmann - Astronomy & Astrophysics, 2024 - aanda.org
Context. HD 209458 b is one of the most studied exoplanets to date. Despite this,
atmospheric characterisation studies yielded inconsistent species detections and …

First comparative exoplanetology within a transiting multi-planet system: Comparing the atmospheres of V1298 Tau b and c

S Barat, JM Désert, JM Goyal, A Vazan… - Astronomy & …, 2024 - aanda.org
The V1298 Tau system is a multi-planet system that provides the opportunity to perform
comparative exoplanetology between planets orbiting the same star. Because of its young …